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1.
Alignment methods for the OPERA drift tube detector / Büttner, B (Hamburg U.) ; Ebert, J (Hamburg U.) ; Ferber, T (Hamburg U. ; DESY) ; Göllnitz, C (Hamburg U.) ; Goloubkov, D (Moscow, ITEP) ; Hagner, C (Hamburg U.) ; Hierholzer, M (Hamburg U. ; Bern U., LHEP) ; Hollnagel, A (Hamburg U.) ; Lenkeit, J (Hamburg U.) ; Rostovtseva, I (Moscow, ITEP) et al.
The goal of the OPERA experiment is to give the first direct evidence for neutrino oscillations in the channel νμ→ντ . The OPERA detector is designed to observe the appearance of tau neutrinos in the originally pure muon neutrino CNGS beam. [...]
2014 - 6 p. - Published in : Nucl. Instrum. Methods Phys. Res., A 747 (2014) 56-61
2.
Discovery of tau neutrino appearance in the CNGS neutrino beam with the OPERA experiment / OPERA Collaboration
The OPERA experiment was designed to search for νμντ oscillations in appearance mode, i.e. by detecting the τ-leptons produced in charged current ντ interactions. [...]
arXiv:1507.01417.- 2015-09-17 - 7 p. - Published in : Phys. Rev. Lett. 115 (2015) 121802 Fulltext: PDF; External links: Interactions.org article; Symmetry Magazine article
3.
Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam / OPERA Collaboration
The OPERA experiment, exposed to the CERN to Gran Sasso νμ beam, collected data from 2008 to 2012. Four oscillated ντ Charged Current interaction candidates have been detected in appearance mode, which are consistent with νμντ oscillations at the atmospheric Δm2 within the "standard" three-neutrino framework. [...]
arXiv:1503.01876.- 2015-06-11 - 11 p. Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint
4.
Observation of nu_tau appearance in the CNGS beam with the OPERA experiment / OPERA Collaboration
The OPERA experiment is searching for nu_mu -> nu_tau oscillations in appearance mode i.e. via the direct detection of tau leptons in nu_tau charged current interactions. [...]
arXiv:1407.3513.- 2014-10-27 - 10 p. - Published in : Prog. Theor. Exp. Phys. 2014 (2014) 101C01 Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint
5.
The Angular Matching Method for the Muon Charge Sign Measurement in the OPERA Experiment / OPERA Collaboration
The long baseline neutrino oscillation experiment OPERA is searching for ντ appearance in the CNGS beam of νμ. The task of the two muon spectrometers of the OPERA detector is to clarify the signature of a muonic τ decay (μ) and to reduce background originating from charmed particles produced in νμ interactions (μ+). [...]
arXiv:1404.5933.- 2016-07-25 - 10 p. - Published in : JINST 11 (2016) P07022 Fulltext: PDF; External link: Preprint
6.
Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays / OPERA Collaboration
The OPERA experiment, designed to perform the first observation of νμντ oscillations in appearance mode through the detection of the τ leptons produced in ντ charged current interactions, has collected data from 2008 to 2012. In the present paper, the procedure developed to detect τ particle decays, occurring over distances of the order of 1 mm from the neutrino interaction point, is described in detail. [...]
arXiv:1404.4357.- 2014-08-07 - 9 p. - Published in : Eur. Phys. J. C 74 (2014) 2986 Article from SCOAP3: PDF; Fulltext: PDF; Springer Open Access article: PDF; External link: Preprint
7.
Measurement of TeV atmospheric muon charge ratio with the full OPERA data / OPERA Collaboration
The OPERA detector, designed to search for ν μ → ν τ oscillations in the CNGS beam, is located in the underground Gran Sasso laboratory, a privileged location to study TeV-scale cosmic rays. For the analysis here presented, the detector was used to measure the atmospheric muon charge ratio in the TeV region [...]
arXiv:1403.0244.- 2014-07-02 - 9 p. Article from SCOAP3: PDF; Fulltext: PDF;
8.
Evidence for νμντ appearance in the CNGS neutrino beam with the OPERA experiment / OPERA Collaboration
The OPERA experiment is designed to search for νμντ oscillations in appearance mode i.e. through the direct observation of the τ lepton in ντ charged current interactions. [...]
arXiv:1401.2079.- 2014-03-05 - 6 p. - Published in : Phys. Rev. D 89 (2014) 051102 Fulltext: PDF; External link: Preprint
9.
New results on νμντ appearance with the OPERA experiment in the CNGS beam / OPERA Collaboration
The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the νμντ channel, via the detection of the τ-leptons created in charged current ντ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. [...]
arXiv:1308.2553.- 2013 - 32 p.
Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint
10.
Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors / LVD and OPERA Collaborations
The purpose of this work is to report the measurement of a time-shift in the OPERA set-up in a totally independent way from Time Of Flight (TOF) measurements of CNGS neutrino events. The LVD and OPERA experiments are both installed in the same laboratory: LNGS. [...]
arXiv:1206.2488.- 2012 - 21 p. - Published in : Eur. Phys. J. Plus 127 (2012) 71 Fulltext: PDF; External link: Preprint

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